Neutral current induced neutrino oscillations in a supernova

Details Neutral current induced neutrino oscillations in a supernova Neutral current induced neutrino oscillations in a supernova

1997-01-16

arxiv.org/abs/hep-ph/9701311v1

Phys.Lett. B396 (1997) 197-200

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, latex, postscript file is also available at ftp://dept.physics.upenn.edu/pub/Kusenko/UPR729T.ps

Scientific paper

10.1016/S0370-2693(97)00121-4

Neutral currents induced matter oscillations of electroweak-active (anti-)neutrinos to sterile neutrinos can explain the observed motion of pulsars. In contrast to a recently proposed explanation of the pulsar birth velocities based on the electron to tau (muon) neutrino oscillations [hep-ph/9606428], the heaviest neutrino (either active or sterile) would have to have mass of order several keV.

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